Round 6: Tossup 1
A type of these objects may have formed inside of Population III “quasi-stars” or through the merger of “intermediate-mass” counterparts. Katie Bouman’s CHIRP algorithm was used to image these objects using very-long-baseline interferometry in the EHT collaboration. These objects' accretion disks may emit large amounts of radiation to power (*) quasars (“KWAY-zars”). One of these objects lies inside the complex radio source Sagittarius A. Most galaxies contain a “supermassive” example of these objects at their center. For 10 points, name these astronomical bodies which are so dense that light cannot escape their gravity. ■END■
ANSWER: black holes [accept supermassive black holes or SMBHs]
<Astronomy — June Yin> | SHOW-ME Four Packet 6
= Average correct buzzpoint
Buzzes
Summary
| Tournament | Edition | Match | Heard | Conv. % | Power % | Neg % | Avg. Buzz |
|---|---|---|---|---|---|---|---|
| Rube Goldberg XIX | 11/20/2025 | ✓ | 16 | 100% | 63% | 6% | 50.25 |
| SHOW-ME Four Nationwide HS | 11/20/2025 | ✓ | 5 | 100% | 80% | 0% | 32.80 |
| SPOOKY IX | 11/20/2025 | ✓ | 5 | 100% | 40% | 20% | 49.40 |